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U.S. Department of Energy
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Electron-positron annihilation and the cosmic X-ray background

Technical Report ·
OSTI ID:5705270
The possibility that the processes responsible for the cosmic X-ray background (CXB) would also produce an e(-)-e(+) annihilation feature is examined. Under the assumption that these proesses are thermal, the absence of a strong e(-)-e( ) annihilation feature places constraints on the compactness (L/R ratio) of these sources. Observations favor souces of small compactness ratio.
Research Organization:
National Aeronautics and Space Administration, Greenbelt, MD (USA). Goddard Space Flight Center
OSTI ID:
5705270
Report Number(s):
N-8327935
Country of Publication:
United States
Language:
English